1 Chapter 2. Optical Fibers Geometrical Optics & Wave Optics in Fiber Loss Dispersion Nonlinearity.
Phys 250 Quantum Optics, Homework #3,...
Transcript of Phys 250 Quantum Optics, Homework #3,...
Phys 250 Quantum Optics, Homework #3, Solutions
1 Problem 2.7
We can express any state as a sum of number states:
|ψ〉 =∑n
Cn |n〉
So...
|ψ′〉 = a |ψ〉
= N∑n
Cn√n |n− 1〉
⇒ 〈ψ′|ψ′〉 = N2∑n
C2nn (due to orthogonality of |n〉)
= N2n
⇒ N =1√n
What about n′?
n′ = 〈ψ′| n |ψ′〉
=1
n
∑n
C2nn(n− 1)
=1
n
(⟨n2⟩− n
)=〈n2〉n− 1
This is not equal to n − 1 unless 〈n2〉 = 〈n〉2, or in other words |ψ〉 is a number state to beginwith! This is because a photon has a higher probability of begin absorbed from a higher excitedstate (stimulated absorption).
2 Problem 2.8
It should be obvious that n = 5.
1
Furthermore:
n′ =〈n2〉n− 1
=12(02) + 1
2(102)
5− 1
= 9?
This may seem strange, but the output from the (normalized) annihilation operator is weighted –the ground state ends up with a weight of 0, hence it does not contribute! (Na |ψ〉 → |9〉, so thefinal state only has a term due to the |10〉 part of the wavefunction.)
Extended explanation: Having a process where you “know” a photon is absorbed implies somesort of “post-selection” is going on – this is actually relatively common in experimental quantumoptics. If a photon was definitely absorbed, the state couldn’t have been in the ground state tobegin with; some how this is equivalent to measuring the state before the absorption process andfinding it to be in the excited state, |10〉 (and ignoring the cases where it wasn’t).
So... how does this work in theory? To conserve energy, an annihilation operator for one modeshould be coupled to a creation operator for another state of the same energy (or several creationoperators for different states whose energy adds up to the original state). A physically sensibleoperator should like more like this:
O ∼ 1 +N(a†b+ a†b
),
where b is the annihilation operator for the second mode, which was previously ignored. The a†bterm is needed for time-reversal symmetry, although it doesn’t really matter here. Our initial statefor the complete system must be something like this:
|ψ〉 =1√2
(|0〉a + |10〉a)⊗ |0〉b ,
where we assume the second mode is in the ground state. We then apply the operator:
O |ψ〉 ∼ (|0〉a + |10〉a)⊗ |0〉b +N√
9 |9〉a ⊗ |1〉b
If we wish to consider only states where we know a photon was absorbed from mode A, we canmeasure mode B and post-select for the states in which it is excited, which looks like:
〈1|b O |ψ〉 ∼ |9〉a
Thus, we recover the effect of an annihilation operator by using a physical operator plus post-selection on a measurement. This implies, by necessity, that we are actually ignoring the part ofthe wavefunction where nothing happened.
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3 Problem 2.10
∑n
n(n− 1) . . . (n− r + 1)Pn =∞∑n=r
n!
(n− r)!Pn
=1
1 + n
∞∑n=r
n!
(n− r)!xn; from 2.145 with x =
n
1 + n
=xr
1 + n
∞∑m=0
(m+ r)!
m!xm; where m = n− r
=xr
1 + nr! (1− x)−(r+1)
=
(r!
1 + n
)(n
1 + n
)r(1 + n)r+1
= r!nr
4 Problem 2.12
For the mixed state, start with (2.229):
P(φ) =1
2π〈φ| ρ |φ〉
=1
4π
(〈φ|0〉 〈0|φ〉︸ ︷︷ ︸
1
+ 〈φ|1〉 〈1|φ〉︸ ︷︷ ︸1
)=
1
2π
For the superposition, start with (2.226):
P(φ) =1
2π
∣∣∣∣∣∑n
e−inφCn
∣∣∣∣∣2
Cn =1√2
{1, eiφ, 0 . . .
}⇒ P(φ) =
1
4π
∣∣1 + ei(θ−φ)∣∣2
=1 + cos(θ − φ)
2π
The mixed state has a flat distribution – this is expected because it is just a statistical mixtureof two number states, and number states have a flat phase distribution (no phase information).A superposition of two number states, however, does have phase information, which results in alumped distribution.
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5 Problem 2.13
The density operator of the thermal state in the number basis is given by (2.138):
ρTh =∑n
Pn |n〉 〈n| ,
but this is just a statistical mixture of number states. As with the last problem, this means thatthe distribution is flat: P(φ) = 1
2π. Of course it has to be, there should be no reason for a thermal
state to prefer a specific phase!
6 Problem 3.1
a† |α〉 = α |α〉
=∑n
Cn√n+ 1 |n+ 1〉
= α∑n
Cn |n〉
⇒ Cn√n+ 1 = αCn+1
⇒ Cn+1 =
√n+ 1
αCn
Which means that Cn monotonically increases with n. This means the state is not normalizableand hence non-physical.
7 Problem 3.4
The easiest way to prove this is to calculate the partial derivative.
4
∂
∂α|α〉 =
∂
∂αe−
αα∗2
∑n
αn√n!|n〉
= −α∗
2|α〉+ e−
αα∗2
∑n
nαn−1
√n!|n〉 (Mathematical reminder:
∂
∂αα∗ = 0)
= −α∗
2|α〉+ e−
αα∗2
∑n
(n+ 1)αn√(n+ 1)!
|n+ 1〉 (Because the n=0 term is 0!)
= −α∗
2|α〉+ e−
αα∗2
∑n
√n+ 1αn√n!
|n+ 1〉
= −α∗
2|α〉+ a† |α〉
∂
∂α〈α| = −α
∗
2〈α|
⇒ ∂
∂α|α〉 〈α| =
(a† − α∗
)|α〉 〈α|
⇒ a† |α〉 〈α| =(α∗ +
∂
∂α
)|α〉 〈α|
The proof of second identity is nearly identical.
8 Problem 3.5
First we calculate⟨X⟩
and⟨X2⟩
:
X1 =1
2
(a+ a†
)⟨X1
⟩α
=1
2〈α| a+ a† |α〉
=1
2(α + α∗) 〈α|α〉
= Re (α)
5
⟨X2
1
⟩α
=1
4〈α| a2 + aa† + a†a+ a†2 |α〉
=1
4〈α| a2 + 2a†a+ 1 + a†2 |α〉
=1
4
(α2 + 2αα∗ + α∗2 + 1
)=
1
4
[(α + α∗)2 + 1
]=
1
4+ Re (α)2
⇒⟨(
∆X1
)2⟩α
=⟨X2
1
⟩α−⟨X1
⟩2
α=
1
4
X2 =1
2i
(a− a†
). . .⟨
X2
⟩α
= Im (α)
⟨X2
2
⟩α
= −1
4〈α| a2 − aa† − a†a+ a†2 |α〉
= −1
4〈α| a2 − 2a†a− 1 + a†2 |α〉
. . .
=1
4+ Im (α)2
⇒⟨(
∆X2
)2⟩α
=⟨X2
2
⟩α−⟨X2
⟩2
α=
1
4
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